US 7218403 B2 Abstract Interferometric scanning method(s) and apparatus for measuring optics either having aspherical surfaces or that produce aspherical wavefronts. A test optic is aligned and moved with respect to a scanning axis relative to the origin of a known spherical wavefront that is generated with a reference surface to intersect the test optic at the apex of the aspherical surface and at radial zones where the spherical wavefront and the aspheric surface possess common tangents. The test surface is imaged onto a space resolving detector to form interferograms containing phase information about the differences in optical path length between the reference surface and the test surface while the axial distance which the test optic moves relative to the spherical reference surface is interferometrically measured. The deviation in the shape of the aspheric surface from its design in a direction normal to the aspheric surface is determined and reported.
Claims(27) 1. An interferometric scanning method for measuring rotationally and non-rotationally symmetric test optics having aspherical surfaces, said method comprising the steps of:
generating at least a partial spherical wavefront along a scanning axis through the use of a decollimator carrying a spherical reference surface positioned along said scanning axis at a known location;
aligning a test optic with respect to said scanning axis and selectively moving said test optic along said scanning axis relative to said spherical reference surface so that said spherical wavefront intersects the test optic at the apex of the aspherical surface and at one or more annular zones where the spherical wavefront and the aspheric surface intersect where their tangents are common;
imaging the test surface onto a space resolving detector to form interferograms containing phase information about the differences in optical path length between the spherical reference surface and the test surface;
interferometrically measuring the axial distance, ν, by which said test optic moves relative to said spherical reference surface; and
analyzing said interferograms to determine the deviation in shape of said aspheric surface compared with its design in a direction normal to the aspheric surface based on the axial distance, ν, and the phase information contained in said interferograms and providing output data of said deviation.
2. The interferometric scanning method of
3. The interferometric scanning method of
4. The interferometric scanning method of
5. The interferometric scanning method of
6. The interferometric scanning method of
7. An interferometric scanning method for measuring rotationally and non-rotationally symmetric test optics having aspherical surfaces, said method comprising the steps of:
generating at least a partial spherical wavefront from a known origin along a scanning axis through the use of a decollimator carrying a spherical reference surface positioned along said scanning axis at a known location with respect to said known origin;
aligning a test optic with respect to said scanning axis and selectively moving said test optic along said scanning axis relative to said spherical reference surface so that said spherical wavefront intersects the test optic at the apex of the aspherical surface and at one or more radial positions where the spherical wavefront and the aspheric surface intersect at points of common tangency;
imaging the test surface onto a space resolving detector to form interferograms containing phase information about the differences in optical path length between the spherical reference surface and the test surface at the one or more positions where points of common tangency occur and generating electrical signals carrying said phase information;
interferometrically measuring the axial distance, ν, by which said test optic moves with respect to said origin; and
determining the deviation in shape of said aspheric surface compared with its design in a direction normal to the aspheric surface based on the axial distance, ν, and the phase information contained in said electrical signals and providing output data of said deviation.
8. The interferometric scanning method of
calculating the optical path length differences, p, between the center of the test optic and the one or more radial positions based on said phase differences contained in said electronic signal; and
calculating the coordinates, z and h, of the aspherical surface wherever said circles of curvature have intersected the aspherical surface at common points of tangency and in correspondence with the interferometrically measured distance, v and calculated optical path lengths, p.
9. The interferometric scanning method of
10. The interferometric scanning method of
11. The interferometric scanning method of
_{0}, the axial separation between the test and reference surfaces, and d, the normal separation of the test and reference surfaces where points of common tangency occur.12. The interferometric scanning method of
_{m }=g−d_{0}, and the measured optical path length difference at the zone of the test optic as p_{m}=d−d_{0}.13. The interferometric scanning method of
_{d }is computed independently of h as p_{d}=p_{d}(νm).14. The interferometric scanning method of
_{m}, is computed as h_{m}=(R_{0}+ν_{m}−p_{m})·√{square root over (p)}_{m}·(2−P_{m}).15. The interferometric scanning method of
_{m}−p_{d }where Δn=fct(Δh_{m}).16. The interferometric scanning method of
17. The interferometric scanning method of
18. The interferometric scanning method of
19. The interferometric scanning method of
_{m}.20. The interferometric scanning method of
_{d}, is computed independently of h as p_{d}=p_{d}(ν_{m}) by eliminating h from the two following equations:by first solving the first equation locally for h and then inserting the result into the second equation.
21. A scanning method for measuring rotationally and non-rotationally symmetric test optics having aspherical surfaces, said method comprising the steps of:
generating at least a partial spherical wavefront from a known origin along a scanning axis through the use of a decollimator carrying a spherical reference surface positioned along said scanning axis upstream of said known origin;
aligning a test optic with respect to said scanning axis and selectively moving said test optic along said scanning axis relative to said known origin so that said spherical wavefront intersects: the test optic at the apex of the aspherical surface and at one or more radial positions where the spherical wavefront and the aspheric surface intersect at points of common tangency;
imaging the test surface onto a space resolving detector to form interferograms containing phase information about the differences in optical path length between the spherical reference, surface and the test surface at the one or more positions where points of common tangency occur and generating electrical signals carrying said phase information;
interferometrically measuring the axial distance, ν, by which said test optic moves with respect to said origin and calculating the optical path length differences, p, between the center of the test optic and the one or more radial positions based on said phase differences contained in said electronic signal,
calculating the coordinates, z and h, of the aspherical surface wherever said circles of curvature have intersected the aspherical surface at common points of tangency and in correspondence with the interferometrically measured distance, ν and calculated optical path lengths, p; and
determining the deviation in shape of said aspheric surface compared with its design in a direction normal to the aspheric surface and providing output data of said deviation.
22. Interferometric scanning apparatus for measuring rotationally and non-rotationally symmetric test optics having aspherical surfaces, said apparatus comprising:
a source for generating a collimated beam of radiation along a scanning axis;
a decollimator carrying a spherical reference surface positioned at a known location along said scanning apparatus to receive said collimated beam and generate at least a partial spherical wavefront;
a precision positioning arrangement for holding and aligning a test optic with respect to said scanning axis and selectively moving said test optic along said scanning axis relative to said spherical reference surface so that said spherical wavefront intersects the test optic at the apex of the aspherical surface and at one or more annular zones where the spherical wavefront and the aspheric surface intersect where their tangents are common;
at least one space resolving detector;
an optical arrangement for imaging the test surface onto said space resolving detector to form interferograms containing phase information about the differences in optical path length between the spherical reference surface and the test surface;
an interferometer for measuring the axial distance; ν, by which said test optic moves relative to said spherical reference surface; and
a control and analysis arrangement for analyzing said interferograms to determine the deviation in shape of said aspheric surface compared with its design in a direction normal to the aspheric surface based on the axial distance, ν, and the phase information contained in said interferograms.
23. The interferometric scanning apparatus of
24. The interferometric scanning apparatus of
25. The interferometric scanning apparatus of
26. The interferometric scanning apparatus of
27. The interferometric scanning apparatus of
Description This application is a continuation-in-part of U.S. patent application Ser. No. 10/180,286 filed on Jun. 26, 2002, now U.S. Pat. No. 6,972,849, in the name of Michael Küchel for “SCANNING INTERFEROMETER FOR ASPHERIC SURFACES AND WAVEFRONTS”, and a continuation-in-part of U.S. patent application. Ser. No. 10/295,479 filed on Nov. 15, 2002, now U.S. Pat. No. 6,879,402, in the name of Michael Küchel for “SCANNING INTERFEROMETER FOR ASPHERIC SURFACES AND WAVEFRONTS”, the entire contents of both of which are incorporated herein by reference. In general, this invention relates to the field of interferometry and, in particular, to the high accuracy measurement of aspherical surfaces and wavefronts in an absolute manner. Aspherical surfaces have become more and more important in modern optical systems because they offer a higher number of parameters for simplifying systems while optimizing their performance. This can lead to systems with less surfaces, less weight, smaller dimensions and higher states of correction, to mention only a view advantages. This is especially true in fields where a high number of optical surfaces are not practical, like in astronomical telescopes or normal incidence reflecting surfaces for the EUV wavelength of 13.6 nm used for lithography tools where it is mandatory to keep the number of surfaces as low as possible. In such cases, there is no choice but to use aspherical surfaces. With demands for high quality performance for complete systems operating in the EUV-regime; the surface errors of reflecting surfaces within such a system must be kept below 0.1 nm, and the measuring accuracy and precision for such errors must be even higher to be able to produce the surfaces in a deterministic manner. In addition, lens surfaces in multi-element lithography lenses operating at wavelengths of 193 nm and 157 nm are made aspherical to lower the number of elements made, which are of rare and expensive materials. In these cases, the departures from a best fitting sphere can be as large as 1000 μm, and the dimensions of such lens surfaces have increased to nearly 500 mm. In an optical system, the function of any of its lens elements is to modify the wavefront transmitted by the individual lens elements according to the optical design of the whole system. If a spherical wave or a plane wave enter such a lens, an aspherical wavefront with a very high departure from the best fitting sphere is produced, depending on the conjugates used in the particular test-configuration. So even the fundamental single lens element with either spherical or aspherical surfaces can only be tested properly if one is able to deal with aspherical wavefronts in a test set-up. Moreover, this ability is very important to testing wavefronts transmitted through lens elements because inhomogeneity of the lens material itself can deteriorate the wavefront even when the surfaces are otherwise free of error. The measurement of aspherical surfaces and wavefronts has been very difficult because of the large departure from the best fitting sphere. With interferometric measurements, high precision is by making the dynamic range of the measurement very small, and for this purpose, the wavefront of the reference wavefront, against which the aspherical wavefront is compared, has to be made aspherically as well to ideally fit the wavefront to be measured completely. In prior art, this has been done either by refractive systems, so called “null-lenses”, or with diffractive elements, so called “computer generated holograms”, which alter a wave of known and measurable shape (spherical or preferably plane wave) as it transits the compensation element to fit the design aspherical surface at the location where it is placed in the test-set up by design. In all these cases, the compensation element must be tested to be sure that the correct wavefront is delivered for comparison. But, it is obvious that the same difficulties exist for this type of testing because, again, an aspherical wavefront is produced. Therefore, only indirect test methods are, applied by, for, instance, measuring the surface of each lens element used in a null system, which is exclusively built with the help of spherical surfaces. Also, the refractive index of the lens material, the lens thickness and the air-spacing of the lenses are measured carefully. Nevertheless, the final accuracy is questionable because of accumulation of measurement errors and the uncertainty of the homogeneity within the lens, material. There are many methods and apparatus in the prior art for measuring aspherical optical surfaces, for example: 1. Contacting and non-contacting stylus based profilers; 2. Contacting and non-contacting stylus based coordinate measuring machines; 3. Spherical wavefront interferometers; 4. Lateral and radial shearing interferometers; 5. Interferometers with null lenses in the measurement path; 6. Scanning spherical wave interferometers; 7. Scanning white light interferometers; 8. Sub-aperture stitching interferometers; 9. Interferometers using computer generated holograms-CGHs; 10. Point diffraction interferometers-PDis; 11. Longer wavelength interferometry; and 12. Two wavelength interferometry. While these techniques have utility for many applications, they are limited in their operational capabilities or precision compared with those needed for today's evolving lithography applications. Contacting and non-contacting stylus based profilers mechanically scan the aspherical surface under test and, therefore, are slow because they measure only a few data points at a time. Slow techniques are very susceptible to measurement errors due to temperature variations during the measurement. The same limitations apply to contacting and non-contacting stylus based coordinate measuring machines. Spherical wavefront interferometers usually require the spacing between the element generating the spherical wavefront and the aspherical surface under test to be scanned thereby increasing the measurement time for the entire surface under test thus introducing another parameter which must be measured, usually by another measurement device, and means, commonly known as stitching, for connecting the data from the various zones which fit as the spacing is scanned. Scanning white light interferometers have many of the same limitations as spherical wavefront interferometers. Lateral and radial shearing interferometers usually measure the slope of the surface under test and thereby introduce measurement errors during the reconstruction of the surface under test via integration of the slopes. This latter type of limitation applies to differential types of profiling techniques as well. Sub-aperture stitching interferometers introduce serious measurement errors in the stitching process. Interferometers using computer generated holograms are susceptible to errors introduced by the CGH and stray Moiré patterns. It is also difficult to calibrate, i.e., know the calibration of the CGH. Point diffraction interferometers are a class of spherical wavefront interferometers, and therefore, have many of the same limitations, as well as poor lateral spatial resolution. None of the prior art approaches is entirely satisfactory since each involves a trade-off that places long lead times on the design of the measurement apparatus and method, requires additional fabrication, increases the difficulty of using and calibrating the measurement apparatus, decreases the accuracy and precision, and greatly increases the cost and delivery time of the aspherical optical element. As a result of certain deficiencies in prior approaches to measuring aspheres, it is a principle object of the present invention to provide a method(s) and apparatus for high accuracy absolute measurement of aspherical surfaces or aspherical wavefronts, either the surface of the final optical part or the wavefront of the final optical lens element in transmission, or by absolutely qualifying the compensation elements for the measurement of aspheres, being either of the refractive, diffractive of reflective type, therefore enabling other, more productive methods for the measurement of the components to be produced in volume. It is another object of this invention to measure the deviation of a given surface, such as an aspheric surface, from its nominal design shape in a direction normal to the surface. It is another object of the present invention to provide method(s) and apparatus for measuring aspherical surfaces and wavefronts with large aspherical departures and surface slopes. It is yet another object of this invention to provide method(s) and apparatus for measuring aspherical surfaces and wavefronts with small departures from spherical surfaces. It is another object of the present invention to provide method(s) and apparatus for measuring aspherical surfaces and wavefronts with large diameters and clear aperture. It is yet another object of the present invention to provide method(s) and apparatus which can be adapted to different measurement purposes and aspherical surfaces and wavefronts in an easy manner. It is still another object of the present invention to provide method(s) and apparatus for measuring aspherical surfaces and wavefronts which can be calibrated absolutely. It is a further object of the present invention to provide method(s) and apparatus which have highly reduced sensitivity to vibrations when measuring aspherical surfaces and wavefronts. It is another object of the present invention to provide method(s) and apparatus which have reduced sensitivity to temperature changes in the measurement of aspherical surfaces and wavefronts. It is yet another object of the present invention to provide method(s) and apparatus which have reduced sensitivity to air turbulence of the gas in the interferometer (measurement) cavity in measuring aspherical surfaces and wavefronts. It is a further object of the present invention to provide method(s) and apparatus that can work with a light source of only a coherence length equal to the aspherical departure. It is yet a further object of the present invention to provide method(s) and apparatus which can also work with wavelengths for which only point detectors exist (UV and IR-range). It is still a further object of the present invention to provide method(s) and apparatus which automatically adjust for the spatial location from where the measurement points are sampled. It is still another object of the present invention to provide method(s) and apparatus which can be adjusted to the spatial resolution required for the measurement. It is yet a further object of the present invention to provide method(s) and apparatus which have reasonable speed of measurement. It is still a further object of the present invention to provide method(s) and apparatus which compute both critical coordinates of the aspherical surface, the radial distance h and the axial distance, z, solely from interferometric measurements and not from the geometrical mapping of the detectors onto the surface. Other objects of the invention will, in part, be obvious and will, in part, appear hereinafter when the detailed description is read with reference to the drawings. In one aspect of the method and apparatus for measuring aspherical surfaces and wavefronts according to the invention, an aspherical: surface is, illuminated with a wavefront that fits the shape of the surface only in some locations, which are at the center and a radial “zone”. In those locations, the surface has the same slope as the illuminating wavefront, i.e., the rays strike the aspherical surface at normal incidence and are reflected back by auto-collimation. It is only in those locations where measurement data points are sampled at the instant of normal incidence. In one variation of the basic principle, the incidence of the rays is not normal to the surface, but the parts of the surface where the actual measurement points are sampled act again as to image the light source with unit magnification, but in a reversed real image. According to the invention, the optical path difference between the center and the “zone” is measured by bringing those rays to interfere with each other and measuring the intensity of the interference. The correct and useful rays for that interference are automatically sampled by the use of an aperture, which is located in the image of the light source. In accordance with the invention, an aspherical test surface is shifted along a scanning axis and as it travels, the same center-part as before is hit by rays, which later enter the aperture, but now the “zone” shifts radially to a new location in correspondence with the axial position of the test surface. In each of the radial “zones” the criterion of normal incidence or, respectively, the imaging criterion of the light-source into the aperture is satisfied. Scanning the aspherical surface axially causes the optical path-difference between the rays from the center and the radially moving zone to change, and the measured intensity of the interference is modulated. With a sliding windowing technique and an appropriate phase-measurement algorithm, the phase-information is extracted from the measured intensity, and from the phase, the optical path difference is calculated. This is done with an algorithm that allows computation of not only the axial position, z, on the aspherical surface, but also the lateral height, h, of each radial “zone”, where the rays are sampled. This is achieved by measuring the optical, path difference of the two rays: (1) from the light source to the zone and back to the sampling aperture and (2) from the light source to the center and back to the sampling aperture interferometrically, while also measuring the scanning of the aspherical surface with the help of an external distance measuring interferometer (DMI). Consequently, two quantities are measured with interferometric precision with the condition of autocollimation satisfied where the light, rays are incident normal to the surface or, equivalently but more generally, that the light source is imaged onto the sampling aperture with magnification=−1. According to another aspect of the invention, the light-source and a corresponding sampling aperture are rings with diameters large enough to be able to resolve the image of the test surface onto the detectors azimuthally, and with a ring width that is small enough to isolate the coherent light from the small areas on the test surface that are probed. It is a special feature of the invention that the detectors are not located in a conjugate to the test surface in the radial direction (i.e., an image of the surface) as is the case for the azimuthal direction, but in a conjugate (i.e., an image) of the light source. With this arrangement, the rays from the center and the “zone” are made to interfere because they are not separated on the detector but made to be on top of each other. The imaging optics behind the sampling aperture is an anamorphic one, but in the sense of radial coordinates, not Cartesian as in the usual case. This special anamorphic imaging is derived by a holographic optical element (similar to a Fresnel zone plate). For detectors, PIN diodes, or the like, having similar sensitivity and frequency response are preferred. According to another aspect of the invention, a test-set up is calibrated absolutely by measuring an aspherical surface of known shape in the same way as an unknown aspherical surface would be probed, i.e., by scanning axially. This known surface could be a parabola, for instance, which can be measured absolutely with the help of a known plane mirror and a known spherical mirror using known procedures available to measure those surfaces in an absolute manner. Another possibility is to use a lens with spherical surfaces used in transmission together with a known auto-collimation mirror. The lens can be measured in transmission beforehand in an absolute manner with the use of other conjugates. According to another aspect of the invention, spherical surfaces, mildly aspheric surfaces, and mildly aspheric surfaces that have more than one departure from a sphere can be measured by using the inventive procedures to locate the zone of contact, unwrap the measured phase values and calculate the phase difference between a zone and the center of the interferogram. In accordance with another aspect of the invention, a scanning interferometric apparatus and associated algorithms operate to measure the deviation of a given surface as, for example, an aspheric surface, with respect to its nominal design value in directions normal to the surface. The structure, operation, and methodology of the invention, together with other objects and advantages thereof, may best be understood by reading the detailed description in conjunction with the drawings in which each part has an assigned numeral that identifies it wherever it appears in the various drawings and wherein: The preferred embodiments together with a associated algorithms will now be described in a more detailed manner. Reference now made to In The axial position of aspherical test surface In the extreme left axial position of the aspherical surface When the surface When the surface The measurement of the surface Lead device The evaluation of the aspherical profile of the surface In K is the best fitting circle with its center on the symmetry—axis z to the rotationally symmetric aspherical curve A. This circle touches the aspherical curve A in the point Q(h,z). The normal to the tangent in Q(h,z) (common to K and to A) cuts the z-axis in the point M(0,R When the center point M(0,R For the following, it is assumed that R The equation for the circle can be written as (See FIG. When the center point is shifted an infinitesimal distance dν, the radius of the circle grows by another infinitesimal quantity dp and the new circle cuts the old circle in the common point Q(h,z). The equation for the new circle is:
To compute the coordinates z and h, Equations (1) and (2) are solved for the quantities z and h to obtain:
It is an important feature of the invention that the axial coordinate z as well as the lateral coordinate h can be computed from the two quantities ν and p, which are both measured by interferometry with very high precision. It is not necessary for the detector to resolve the radial coordinate h, where the circle and the aspherical curve coincide at the point of common tangency. Having described how to calculate the local slope and its position on the aspheric surface through the simple expediency of interferometrically measuring the axial separation between the focus point After evaluation of p(ν), the derivative p′(ν) is computed as well by fitting a function (for instance a polynomial or a higher order piecewise spline function) to a portion of p=p(ν) with ν Now slit Assuming an aspherical deviation of 0.5 mm from the sphere which cuts in 3 points, the aspherical deviation from the sphere which fits the aspherical curve in the apex might be 3 mm, for instance as shown in To improve measurement speed then, use can be made of multiple detectors instead of the slit aperture Behind the ring-shaped aperture Each of the detectors If 60 detectors are arranged in a circle, and the same azimuthal resolution as before is assumed, 360 positions at the circumference of the surface The foregoing methods of detecting the phase values from the intensity measurements, according to Equation (5) have the drawback that variations in the mean intensity A(ν), or in the modulation B(ν), influence the computed values of p(ν). Therefore, it must be assured that such variations will not take place. Due to the high frequency structure that aspherical surfaces might show and due to the “knife-edge like” optical arrangement with a very small ring aperture (like a round slit), this assumption might not be satisfied in all situations. Therefore, it might be necessary to think of alternative ways for phase-extraction from the measurements with the arrangements given with One approach is to use different polarization stages for the beam at the center of the asphere and the beam at the zone. This can be accomplished by an extra-element inserted in the space between lens When the center part of the beam transverses the quarter-wave plate twice, the linearly-polarized wave has its plane of polarization rotated by 90°. Thus, the two beams are “encoded” by their polarization states, and the relative phase between the beams can be shifted by polarization controlling optical means. There are at least two possibilities which might be applied, which are given in In In The principle of phase-shifting by polarization is well known: two linearly polarized beams with orthogonal polarization directions transit a properly oriented quarter-wave plate and then transit a rotating, half-wave plate. Along with the rotation of this plate, phase modulation takes place. The beams can finally interfere when they are made the same polarization with the help of a polarizer. In In In the following -
- Testing (i.e., finding the wavefront-errors to be used as a correction-matrix in the final application of the null-lens) the refractive null lens or the diffractive CGH;
- Testing the aspherical surface;
- Calibrating the test-set-up with the help of an aspherical surface, which is known a priori. This possibility is described later in greater detail;
- Qualifying a refractive null-lens, as it is described in and needed for the task described in U.S. Provisional Patent Application No. 60/299,512 filed in the name of Carl A. Zanoni on Jun. 20, 2001 for METHOD FOR MEASURING ASPHERICAL OPTICAL SURFACES and later converted in U.S. patent application Ser. No. 10/152,075 filed in the name of Carl A. Zanoni on May 21, 2002 for APPARATUS AND METHOD FOR MEASURING ASPHERICAL OPTICAL SURFACES AND WAVEFRONTS; now U.S. Pat. No. 6,771,375 issued on Aug. 3, 2004, and
- Testing lenses in transmission in different configurations.
The arrangements of In all the foregoing embodiments, it is possible to scan over the surface or wavefront in the radial direction by axially shifting one auto-collimation element. Together with this shift, the heterodyne frequency for the phase-measurement is delivered automatically. In all cases other than those of Three possibilities for calibrating test set-ups are shown in Therefore, the final accuracy of the measurements is based on the quality with which a special aspherical surface, like a parabola, can be performed. It should be mentioned that the measurement of a parabola can be related to the measurement of a plane and a sphere, and both can be performed absolutely. Another candidate for calibration purposes is a hyperbola, which can be tested with the help of two spheres. Also, a lens in transmission together with a sphere for auto-collimation can be used. In addition, lenses exist which deliver a stigmatic wavefront in a special configuration (and can be tested with solely spherical wavefronts) and deliver a strong aspherical wavefront in different configuration, which can be used for calibration. Reference is now made to As best seen in An intermediate image of the surface under test occupies the intervening space As before, a surface under test Where it is important to reduce the effects of coherent artifacts, the illumination system may be replaced by a ring shaped source such as that shown and described in connection with Having described the major structural differences with this embodiment, its principal and method of operation will now be described with reference to When mild aspherical surfaces are illuminated with a spherical wavefront in a Fizeau cavity, provided as here, with a spherical reference surface It will be appreciated that, when the interferograms thus formed are analyzed, the phase in the center of the surface and also in the zone, where the rays are nearly perpendicular, the departure from the fitting sphere is either concave or convex as illustrated in After establishing the gap value, the measurement sequence is begun as shown in Reference is now made to The steps followed in the flow chart of Secondly, the part is scanned by an amount Δν=fct(Δh) where the steps for Δν are preferably chosen using the following procedure. The amount of steps to be performed in ν, i.e., the steps Δν can be pre-calculated from a curve ν=ν(h), where ν is the scan distance and h is the radius of the zone. Such a curve is given in Next, measurements at the apex of the part→d To take measurement data at the apex includes several steps. The scan-position of the part, i.e., the ν-values are measured coarsely with an external measurement device, i.e., with a laser distance interferometer. On the other hand, a phase-measurement is made at the apex and the phase steps of 2π are removed. For this procedure the “center” of the field of view must be defined, because here the phase-unwrapping must start and also the value of the phase must be finally taken. The center of the field of view, shortly called “the center”, can be defined by the center of a best fitting circle through the “zone”. This is explained in detail hereafter. After the phase-unwrapping, Zernike functions are fitted to the measured phase values to reduce measurement noise. For these Zernike functions, the rotationally symmetrical functions, as well as all coma terms are used. Finally, the value at the center of the Zernike phase map is used as the measurement value. This gives the fringe fraction of the measurement by multiplying the phase-fraction by λ/4π. In addition, the fringe order number must be added, and this is derived from the distance measuring interferometer (DMI) readings and “tracking” of order numbers. It may be possible for the phase-values measured directly at the apex of the part to be corrupted heavily by ghosts form the optics of the mainframe. In such a case, the accuracy might be not sufficient. If so, use may be made of the double phase shift method described in previously referenced U.S. Pat. No. 6,717,680 to solve this problem. Here, the reference surface is shifted in addition to the test surface, and the phases in the resultant 3 cavities: (1) test surface with reference surface; (2) test surface with ghost; and (3) reference surface with ghost are derived separately by solving a linear system of equations. Only the phase of cavity (1) has to be calculated explicitly. The fourth step of taking measurement data at the zone is also done in several steps, which also include a fitting procedure, as with the apex. Here, a zone is predicted where measurement values can be expected. This zone prediction is performed with the help of the design values. Second, the measured phase fractions for the zone of interest are unwrapped to get a continuous phase-surface at the zone, which is similar to a torus. Third, a polynomial of the following form is fitted:
The two additional terms P The method for finding this lateral shift by using P - 1. Choose a “rough center” for the calculations, i.e., some initial position on the phase-map in detector coordinates, where the real “center”, which is the center of the red circle, is roughly assumed.
- 2. Trace some radial lines in equal angle, increments with azimuth angle θ through this center (maybe 36), and calculate the phase-values along these lines around the “zone”.
- 3. Find the extreme values φ(x,y)=φ(θ) of the phase.
- 4. Calculate a best fitting circle though the coordinate points x,y of the extreme values: center point (x—blue, y—blue) and radius (r—blue).
- 5. Fit functions a sin θ and b cos θ through the values φ(θ); find the extreme values p
_{1}−p=p−p_{2 }from p_{1}−p=√{square root over (a^{2}+b^{2})} and the direction β of the shift from the β=arctan (a/b). - 6. The center for the red circle is found by x—red=x—blue+Δx and y—red=y—blue+Δy where Δx and Δy are computed from Eq. (8) as follows:
- 7. Compute the phase values on the “red circle” by interpolation as done before (combination of Lagrange-Polynomials and cos and sin—function with a well defined coordinate center.
Referring back now to the flow chart of The sixth step involves calculating the value of p(θ,ν): p Referring to step 7, a most important feature of the method is that the work is done in two “coordinate systems” as in two regimes; they are the p,ν system and the z,h system. The equations give the connection between them. Now, a measured surface error is expressed in the normal direction as a function of h. The quantity p is measured in the normal direction to the surface automatically by the “self adaptive” feature of the method. Therefore, an error in the normal direction is an error in p, i.e., it is by definition the deviation of the measured value from the “design value”. But, now the “design value” for p at this location is required. So, it is very important to understand, that this location is not defined by h, but by ν As the eight step, the error in the normal direction is computed: Δn=p Another equation is used in the box of step 9. In this equation, not only the quantity p=p(ν) is needed, but also the first derivative of that function; dp/dν=dp(ν)/dν. The differentiation can be done locally on the measured function, and it is very fortunate to use the averaged value of the function, p=p(ν), over all azimuthal positions for that. Thus, a very robust and numerically stable result is gained. We refer here to Eq. (7) where, by the fitting procedure a mean value for p is automatically gained and can be combined with ν. It is also important to use the measured value for R Step 10 involves combining steps 8 and 9. In accordance with step 11, it is very useful to rotate the part by 180 degrees (reversal) and perform a second scan to eliminate repeatable errors introduced by tip, tilt, and straightness errors in slide Step 12 ends the measurement sequence. While the method of the invention works well for 90% of the part, near the inner 10% of the part special care needs to be taken. This is because ν, p, and p′ are all very small, so the prior equation for h can result in some uncertainty. Therefore, for this region, it is preferred to calculate has a function of the measured value ν As stated earlier, the fundamental problem to be solved is to measure the deviation of the aspheric surface The h-value of the part (lateral location of the extreme value at the zone) is related to an h For establishing the relation between the h and the h Having calculated the radius h of the (average) zone in both coordinate systems, i.e., having established a table with h After having done this, the imaging conditions of the interferometer set-up are known from experiment also in the vicinity of the vertex by using the polynomial of Eq. 14). Now using “conventional” Fizeau interferometry, a certain value of ν (for instance also for ν=0) can be related to the measured image height h To derive the correct equation refer again to From _{1} ^{2}+(R _{0} +ν−z*)^{2})} (19)_{2} _{2} (20)→d _{1} =R _{2} −√{square root over (h* (21)^{2}+(R_{0}+ν−z*)^{2})}This value d The design equation gives z*=fct(h*), but the problem is that only h*
The other equation, that is solved simultaneously for (h,z) is the design equation for the aspherical surface:
When the iteration comes to a stationary value h, this value is then h*. Inserting that value h* into either Eqs. (21) or (22) gives then z*. These values then can be inserted into Eq. (20) to get the design value for d Again, the error in the normal direction to the surface is needed. As the measurements are all relative, no absolute value for d Therefore the phase difference (d This result is now compared with the equivalent design value around the zone, which results in the following difference:
_{2}+(R _{0} +ν−p _{d})=(R _{0} +ν−P _{d})−√{square root over (h* (26)^{2}+(R_{0}+ν−z*)^{2})}where p _{d }means design. This is essentially what is shown in For the starting value for h for the iteration of Eq. (23), use is made of the coordinate h
Having described the embodiments and operation of the invention, variations will occur to others based on its teachings. Therefore, it is intended that all such variations be within the scope of the invention. Patent Citations
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